We have obtained 462 new V and R observations of the RR Lyrae star GV Andromedae. Our data set is consistent with a primary period of 0.528092 days; however, the light curve of GV And cannot be well described by a single period. We conclude that GV And demonstrates the Blazhko effect with a Blazhko period of approximately 32 days
Aims.Extensive photometry of RR Lyr was obtained over a 421-day interval in 2003–2004, covering mor...
Aims.Extensive photometry of RR Lyr was obtained over a 421-day interval in 2003–2004, covering mor...
The cause of the Blazhko effect, the long-term modulation of the light and radial velocity curves of...
We have obtained 462 new V and R observations of the RR Lyrae star GV Andromedae. Our data set is ...
We have obtained 551 new V and R observations of the RR Lyrae star DR Andromedae. Our data set is ...
We have obtained 551 new V and R observations of the RR Lyrae star DR Andromedae. Our data set is ...
We have obtained 615 new V and R observations of the RR Lyrae star FM Per. A period search identif...
We have obtained 615 new V and R observations of the RR Lyrae star FM Per. A period search identif...
Our survey consists of photometric observations of 107 RR Lyrae stars of type RR$\sb{\rm ab}$ and ha...
Our survey consists of photometric observations of 107 RR Lyrae stars of type RR$\sb{\rm ab}$ and ha...
Our survey consists of photometric observations of 107 RR Lyrae stars of type RR$\sb{\rm ab}$ and ha...
With increasingly accurate data on RR Lyrae stars we find that the Blazhko effect may be a rule rath...
Aims. Extensive photometry of RR Lyr was obtained over a 421-day interval in 2003-2004, covering mor...
The All Sky Automated Survey (ASAS) monitors bright stars (8 < V < 14 mag) south of declinatio...
The All Sky Automated Survey (ASAS) monitors bright stars (8 mag < V < 14 mag) south of declination ...
Aims.Extensive photometry of RR Lyr was obtained over a 421-day interval in 2003–2004, covering mor...
Aims.Extensive photometry of RR Lyr was obtained over a 421-day interval in 2003–2004, covering mor...
The cause of the Blazhko effect, the long-term modulation of the light and radial velocity curves of...
We have obtained 462 new V and R observations of the RR Lyrae star GV Andromedae. Our data set is ...
We have obtained 551 new V and R observations of the RR Lyrae star DR Andromedae. Our data set is ...
We have obtained 551 new V and R observations of the RR Lyrae star DR Andromedae. Our data set is ...
We have obtained 615 new V and R observations of the RR Lyrae star FM Per. A period search identif...
We have obtained 615 new V and R observations of the RR Lyrae star FM Per. A period search identif...
Our survey consists of photometric observations of 107 RR Lyrae stars of type RR$\sb{\rm ab}$ and ha...
Our survey consists of photometric observations of 107 RR Lyrae stars of type RR$\sb{\rm ab}$ and ha...
Our survey consists of photometric observations of 107 RR Lyrae stars of type RR$\sb{\rm ab}$ and ha...
With increasingly accurate data on RR Lyrae stars we find that the Blazhko effect may be a rule rath...
Aims. Extensive photometry of RR Lyr was obtained over a 421-day interval in 2003-2004, covering mor...
The All Sky Automated Survey (ASAS) monitors bright stars (8 < V < 14 mag) south of declinatio...
The All Sky Automated Survey (ASAS) monitors bright stars (8 mag < V < 14 mag) south of declination ...
Aims.Extensive photometry of RR Lyr was obtained over a 421-day interval in 2003–2004, covering mor...
Aims.Extensive photometry of RR Lyr was obtained over a 421-day interval in 2003–2004, covering mor...
The cause of the Blazhko effect, the long-term modulation of the light and radial velocity curves of...
Add to ORKG